Extragalactic Multi-Band Exploration of Red Supergiants (EMBERS): Pipeline, Source Classification, and Bolometric Properties of 101,219 Red Supergiants from James Webb Space Telescope Imaging
Abstract
The evolution of red supergiants (RSGs), especially in their final stages before exploding as hydrogen-rich Type II supernovae (SNe), remains poorly understood, owing to small samples of well-characterized stars in the Local Group. We present the largest population study of RSGs to date using ∼105 stars with bolometric parameters inferred from archival James Webb Space Telescope/Near-Infrared Camera (NIRCam) imaging of 15 galaxies within 20 Mpc. We also present jwst123, a newly-developed general-purpose NIRCam reduction and photometry pipeline, and its application to our set of 15 galaxies. We build a simulation-based parameter inference framework to rapidly fit multi-band photometry of ∼1.5 million luminous stars in milliseconds per source. Using clustering in the effective temperature (Teff)-luminosity (log L/L⊙)-dust optical depth (τV) phase space, we introduce a novel method to select RSGs with high completeness and purity. Leveraging the scale of our catalog, we find that the dustiest RSGs prefer metal-rich hosts, and RSG luminosities correlate with host specific star formation rate, suggesting that environment shapes RSG evolution. While most selected RSGs agree with theoretical stellar evolution tracks, we identify a new population of 1,669 RSGs that are heavily dust-enshrouded (τV>4), overluminous (log(L/L⊙)>5.55), or anomalously cool (Teff<3000 K), including analogs of known SN progenitors. Our catalog provides a population-scale baseline for understanding massive stellar evolution and connecting field RSGs to dusty progenitors of Type II SNe.
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BibTeX
@misc{suresh2026extragalactic,
title = {{Extragalactic Multi-Band Exploration of Red Supergiants (EMBERS): Pipeline, Source Classification, and Bolometric Properties of 101,219 Red Supergiants from James Webb Space Telescope Imaging}},
author = {Aswin Suresh and Charles D. Kilpatrick and Wen-fai Fong and Maria R. Drout and Daichi Hiramatsu and Luca Izzo and Wynn V. Jacobson-Galán and Armin Rest and Samaporn Tinyanont},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2609.19344},
eprint = {2609.19344},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.19344},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Extragalactic Multi-Band Exploration of Red Supergiants (EMBERS): Pipeline, Source Classification, and Bolometric Properties of 101,219 Red Supergiants from James Webb Space Telescope Imaging
AU - Aswin Suresh
AU - Charles D. Kilpatrick
AU - Wen-fai Fong
AU - Maria R. Drout
AU - Daichi Hiramatsu
AU - Luca Izzo
AU - Wynn V. Jacobson-Galán
AU - Armin Rest
AU - Samaporn Tinyanont
PY - 2026
DA - 2026/09/16
PB - arXiv
DO - 10.48550/arxiv.2609.19344
UR - https://arxiv.org/abs/2609.19344
AB - The evolution of red supergiants (RSGs), especially in their final stages before exploding as hydrogen-rich Type II supernovae (SNe), remains poorly understood, owing to small samples of well-characterized stars in the Local Group. We present the largest population study of RSGs to date using ∼10^5 stars with bolometric parameters inferred from archival James Webb Space Telescope/Near-Infrared Camera (NIRCam) imaging of 15 galaxies within 20 Mpc. We also present jwst123, a newly-developed general-purpose NIRCam reduction and photometry pipeline, and its application to our set of 15 galaxies. We build a simulation-based parameter inference framework to rapidly fit multi-band photometry of ∼1.5 million luminous stars in milliseconds per source. Using clustering in the effective temperature (T_eff)-luminosity (log L/L_⊙)-dust optical depth (τ_V) phase space, we introduce a novel method to select RSGs with high completeness and purity. Leveraging the scale of our catalog, we find that the dustiest RSGs prefer metal-rich hosts, and RSG luminosities correlate with host specific star formation rate, suggesting that environment shapes RSG evolution. While most selected RSGs agree with theoretical stellar evolution tracks, we identify a new population of 1,669 RSGs that are heavily dust-enshrouded (τ_V>4), overluminous (log(L/L_⊙)>5.55), or anomalously cool (T_eff<3000 K), including analogs of known SN progenitors. Our catalog provides a population-scale baseline for understanding massive stellar evolution and connecting field RSGs to dusty progenitors of Type II SNe.
ER -